Titan's polar surface is dotted with hundreds of lacustrine depressions. Based on the
hypothesis that they are karstic in origin, we aim at determining the efficiency of surface …

The shorelines of Titan's hydrocarbon seas trace flooded erosional landforms such as river
valleys; however, it is unclear whether coastal erosion has subsequently altered these …

There are few identifiable impact craters on Titan, especially in the polar regions. One
explanation for this observation is that the craters are being destroyed through fluvial …

We present a geomorphologic map of Titan's polar terrains. The map was generated from a
combination of Cassini Synthetic Aperture Radar (SAR) and Imaging Science Subsystem …

The Cassini RADAR mapper has imaged elevated mountain ridge belts on Titan with a
linear-to-arcuate morphology indicative of a tectonic origin. Systematic geomorphologic …

Abstract Cassini Synthetic Aperture Radar (SAR) images of Titan's surface revealed river
networks strikingly similar to those on Earth. However, Cassini SAR has low spatial …

Detailed analyses of slopes and arcuate planform morphologies of Titan's equatorial
mountain ridge belts are consistent with formation by contractional tectonism. However …

River valleys have been observed on Titan at all latitudes by the Cassini‐Huygens mission.
Just like water on Earth, liquid methane carves into the substrate to form a complex network …

Evidence for tectonic activity on Titan is provided by the presence of eroded mountain
ranges. Xanadu is an equatorial region of Titan characterized by a complex topography …